Paper Citation Record · LEDGER

Holographic motivations and observational evidence for decreasing dark energy

As of 20 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 6 inbound Pith citation observations for arXiv:2406.02688.

A citation records a reference. It does not transfer a finding from one paper to another.

pith.paper-citation-record.v1
2406.02688 v1

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measured 6 of 6 standing notices

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Source: scholarly_work_events, retraction_status_cache, observed 2026-08-19T06:32:44.657259+00:00

measured 6 of 6 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-15T19:15:54.807500Z

measured 0 of 1 external citation measurements

A source-named dated measurement, never combined with another source.

Source: arxiv_reference, observed 2026-05-13T17:38:03.039771Z

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Outbound references

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Pith citing papers

Observation 4f07d7a6-0744-469f-ae3f-851620b86ad0 · inbound

Prepare inflationary universe via the Euclidean charged wormhole cites this paper.

Prepare inflationary universe via the Euclidean charged wormhole Holographic motivations and observational evidence for decreasing dark energy

Reference 83

Resolution: unresolved; no resolver link, observed 2026-08-12T15:54:21.318178Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation fdec4fe2-7f45-4413-8e32-5f67fe94c6b5 · inbound

Holographic black hole cosmologies cites this paper.

Holographic black hole cosmologies Holographic motivations and observational evidence for decreasing dark energy

Reference 1

Resolution: unresolved; no resolver link, observed 2026-08-12T15:07:31.922732Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 323df823-f056-4057-890a-4082fef76a36 · inbound

Is excess smoothing of Planck CMB ansiotropy data partially responsible for evidence for dark energy dynamics in other $w(z)$CDM parametrizations? cites this paper.

Is excess smoothing of Planck CMB ansiotropy data partially responsible for evidence for dark energy dynamics in other $w(z)$CDM parametrizations? Holographic motivations and observational evidence for decreasing dark energy

Reference 73

Resolution: unresolved; no resolver link, observed 2026-08-10T22:00:59.957264Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 6c127850-882e-4c20-84f9-3960ce529a7d · inbound

Standardizing a larger, higher-quality, homogeneous sample of reverberation-mapped H$\beta$ active galactic nuclei using the broad-line region radius-luminosity relation cites this paper.

Standardizing a larger, higher-quality, homogeneous sample of reverberation-mapped H$\beta$ active galactic nuclei using the broad-line region radius-luminosity relation Holographic motivations and observational evidence for decreasing dark energy

Reference 130

Resolution: unresolved; no resolver link, observed 2026-08-15T19:15:54.807500Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation a3cee634-8dc9-4d01-a580-9b92bbfb1650 · inbound

Updated observational constraints on $\phi$CDM dynamical dark energy cosmological models cites this paper.

Updated observational constraints on $\phi$CDM dynamical dark energy cosmological models Holographic motivations and observational evidence for decreasing dark energy

Reference 25

Resolution: unresolved; no resolver link, observed 2026-08-04T13:43:12.216650Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 0fe925e6-a312-4ac0-81b8-19eb76ea570d · inbound

Is the $w_0w_a$CDM cosmological parameterization evidence for dark energy dynamics partially caused by the excess smoothing of Planck PR4 CMB anisotropy data? cites this paper.

Is the $w_0w_a$CDM cosmological parameterization evidence for dark energy dynamics partially caused by the excess smoothing of Planck PR4 CMB anisotropy data? Holographic motivations and observational evidence for decreasing dark energy

Reference 19

Resolution: verified exact; arxiv_id, observed 2026-05-13T17:38:03.041277Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.